Physics
Scientific paper
Aug 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnt...16..256g&link_type=abstract
Kinematika i Fizika Nebesnykh Tel, vol. 16, no. 3, p. 256-260
Physics
Scientific paper
Peculiarities of two cometary groups revealed earlier are investigated. Comets of the first group are characterized by large perihelion distances, large inclinations of orbits, correlation between q and B', concentration of nodes and perihelia in two opposite intervals. These peculiarities do not contradict the hypothesis of planet-source of this group, and some of them agree quite well with it. The second group is similar to the first one, and it is likely to be genetically related to it.
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